Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
3.8581 7.3476 0.0054 26.8872 -129.8025 2.6413841 35.381 TRIG_00726885
Foreground time interval of the image:
-0.424 12.933 (delta_t = 13.357 [sec])
Background time interval of the image:
-182.067 -0.424 (delta_t = 181.643 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
- 4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
- 5) Time of each bin is in the middle of the bin.
1 s binning
From T0-310 s to T0+310 s
From T100_start - 20 s to T100_end + 30 s
Full time interval
64 ms binning
Full time interval
From T100_start to T100_end
From T0-5 sec to T0+5 sec
16 ms binning
From T100_start-5 s to T100_start+5 s
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
- 3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from -0.424 sec. to 30.828 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.75420 ( -0.0858496 0.0867845 )
Norm@50keV : 7.12195E-03 ( -0.00034332 0.000341194 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.69 using 59 PHA bins.
# Reduced chi-squared = 0.7139 for 57 degrees of freedom
# Null hypothesis probability = 9.494515e-01
Photon flux (15-150 keV) in 31.25 sec: 0.964550 ( -0.044445 0.04453 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.05348e-06 ( -1.02511e-07 1.03223e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.424 sec. to 30.828 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62694 ( -0.337746 0.202226 )
Epeak [keV] : 139.007 ( -69.7813 -139.007 )
Norm@50keV : 8.29815E-03 ( -0.00157229 0.00404023 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.23 using 59 PHA bins.
# Reduced chi-squared = 0.7183 for 56 degrees of freedom
# Null hypothesis probability = 9.445994e-01
Photon flux (15-150 keV) in 31.25 sec: 0.956697 ( -0.048383 0.048243 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.70817e-06 ( -1.55063e-07 6.51662e-08 ) ergs/cm2
Band function
Time interval is from -0.424 sec. to 30.828 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.4561 ( )
R^2/D10^2 : 0.193391 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 161.53 using 59 PHA bins.
# Reduced chi-squared = 2.8339 for 57 degrees of freedom
# Null hypothesis probability = 6.176860e-12
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.988e-07 1.661e-08
25- 50 6.530e-07 3.359e-08
50-150 6.242e-07 6.203e-08
15-150 1.476e-06 7.688e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 115.633 (-19.7766 32.4504)
Norm : 4.09539 (-0.264596 0.262828)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.94 using 59 PHA bins.
# Reduced chi-squared = 0.7534 for 57 degrees of freedom
# Null hypothesis probability = 9.161796e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.338e-07 2.839e-08
25- 50 5.933e-07 3.453e-08
50-150 1.039e-06 2.716e-07
15-150 1.966e-06 3.075e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.60963 (-0.905335 0.968849)
R1^2/D10^2 : 1.42672 (-0.539676 1.01058)
kT2 [keV] : 25.0775 (-3.95775 5.98714)
R2^2/D10^2 : 1.15827E-02 (-0.00616186 0.0105134)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.76 using 59 PHA bins.
# Reduced chi-squared = 0.7593 for 55 degrees of freedom
# Null hypothesis probability = 9.058067e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.331e-07 4.831e-08
25- 50 5.832e-07 6.844e-08
50-150 1.094e-06 2.141e-07
15-150 2.010e-06 3.005e-07
Peak spectrum fit
Power-law model
Time interval is from 0.112 sec. to 1.112 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55762 ( -0.203619 0.208171 )
Norm@50keV : 1.77416E-02 ( -0.00207611 0.00204354 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.16 using 59 PHA bins.
# Reduced chi-squared = 0.9327 for 57 degrees of freedom
# Null hypothesis probability = 6.197973e-01
Photon flux (15-150 keV) in 1 sec: 2.25103 ( -0.24658 0.24696 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66863e-07 ( -2.13573e-08 2.16668e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.112 sec. to 1.112 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.25245 ( -1.03724 0.0911074 )
Epeak [keV] : 92.3761 ( )
Norm@50keV : 7.64450E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.17 using 59 PHA bins.
# Reduced chi-squared = 0.9316 for 56 degrees of freedom
# Null hypothesis probability = 6.206574e-01
Photon flux (15-150 keV) in 1 sec: 2.25090 ( -0.24679 0.24679 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.68043e-07 ( -2.80295e-08 1.06675e-08 ) ergs/cm2
Band function
Time interval is from 0.112 sec. to 1.112 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 14.0167 (-2.08029 2.55961)
R^2/D10^2 : 0.308675 (-0.136372 0.236185)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 82.14 using 59 PHA bins.
# Reduced chi-squared = 1.441 for 57 degrees of freedom
# Null hypothesis probability = 1.628854e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.281e-08 2.915e-09
25- 50 4.770e-08 7.580e-09
50-150 6.174e-08 1.488e-08
15-150 1.222e-07 1.821e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.345 (-81.6702 -199.363)
Norm : 9.11418 (-0.989035 0.989293)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.74 using 59 PHA bins.
# Reduced chi-squared = 0.9603 for 57 degrees of freedom
# Null hypothesis probability = 5.604229e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.269e-08 1.265e-08
25- 50 4.366e-08 2.380e-08
50-150 9.575e-08 5.240e-08
15-150 1.621e-07 8.375e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.74451 (-1.87292 4.2498)
R1^2/D10^2 : 10.7066 (-9.21223 106.801)
kT2 [keV] : 22.7343 (-5.9598 33.4197)
R2^2/D10^2 : 5.00425E-02 (-0.0456119 0.126822)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.70 using 59 PHA bins.
# Reduced chi-squared = 1.031 for 55 degrees of freedom
# Null hypothesis probability = 4.114953e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.572e-08 1.319e-08
25- 50 3.743e-08 1.340e-08
50-150 9.849e-08 4.980e-08
15-150 1.616e-07 4.744e-08
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69463 ( -0.0805748 0.0812348 )
Norm@50keV : 1.25234E-02 ( -0.000566619 0.000564191 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.44 using 59 PHA bins.
# Reduced chi-squared = 0.6743 for 57 degrees of freedom
# Null hypothesis probability = 9.719256e-01
Photon flux (15-150 keV) in 13.36 sec: 1.66013 ( -0.0738885 0.0740235 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.54979e-06 ( -7.37527e-08 7.41499e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.46823 ( -0.327137 0.262875 )
Epeak [keV] : 113.676 ( -41.2237 -113.676 )
Norm@50keV : 1.63692E-02 ( -0.00418938 0.00753863 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.84 using 59 PHA bins.
# Reduced chi-squared = 0.6578 for 56 degrees of freedom
# Null hypothesis probability = 9.776208e-01
Photon flux (15-150 keV) in 13.36 sec: 1.63682 ( -0.07987 0.07991 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.51782e-06 ( -8.59582e-08 8.57044e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 5.69e-07
S(50-100 keV) = 6.75e-07
T90 vs. Hardness ratio plot
T90 = 24.8959999680519 sec.
Hardness ratio (energy fluence ratio) = 1.18629
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.22302
Count Ratio (50-100 keV) / (15-25 keV) = 0.7458
Mask shadow pattern
IMX = -3.245836867057915E-01, IMY = 3.895425678363345E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
Spacecraft aspect plot
Bright source in the pre-burst/pre-slew/post-slew images
Pre-burst image of 15-350 keV band
Time interval of the image:
-182.067400 -0.424000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
48.6719 -13.8462 2.1 47.3 148.4 3.6177 5.4 ------ UNKNOWN
1.6581 -26.5637 2.6 57.2 -154.1 5.7424 4.4 ------ UNKNOWN
333.7240 41.7137 3.1 43.2 -53.9 2.2483 3.7 ------ UNKNOWN
331.5570 37.3421 4.5 44.8 -60.3 2.5979 2.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.424000 12.932600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
53.9613 -7.7836 2.5 45.3 137.6 0.8786 4.6 ------ UNKNOWN
3.8581 7.3476 0.3 26.9 -129.8 2.6411 35.4 497.6 UNKNOWN
322.7611 50.3082 2.9 51.4 -43.0 1.0496 4.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
63.932600 955.532600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.1852 38.5199 12.7 46.0 -19.2 -1.1941 -0.9 11.9 Cyg X-2
31.8559 30.6752 4.2 35.1 67.1 3.7730 2.8 ------ UNKNOWN
7.9870 16.2403 2.4 9.8 46.5 2.7619 4.9 ------ UNKNOWN
339.5976 17.2480 2.4 25.6 -42.6 3.2544 4.9 ------ UNKNOWN
359.4492 -49.7306 4.2 57.2 -154.2 12.9046 2.8 ------ UNKNOWN
327.9594 -9.4437 4.0 39.5 -92.2 9.2569 2.9 ------ UNKNOWN
331.4498 -19.2391 4.1 41.6 -107.9 8.7400 2.9 ------ UNKNOWN
Plot creation:
Thu Jan 5 10:41:58 EST 2017